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T. Suda

55 papers hereh-index 212k citations115 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author1
  • first author14
  • middle author33
  • last author7

Across the 55 of 55 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR28
  • astro-ph.GA16
  • astro-ph9
  • astro-ph.HE1
  • nucl-th1
same name
  • T. Suda — 8 papers, h 4
  • T. Suda — 5 papers, h 9
  • T. Suda — 4 papers, h 22
  • T. Suda — 4 papers, h 4
  • T. Suda — 3 papers, h 44
  • T. Suda — 2 papers, h 32

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20042026
most citedThe Stellar Abundances for Galactic Archeology (SAGA) Database - Compilation of the Characteristics of Known Extremely Metal-Poor Stars

436 citations · 2.4k across the 53 of their papers we have counts for

collaborators
Showing 2006Show all

3 papers · 1 filter

astro-ph2006★ 14 cited

Surface pollution of main-sequence stars through encounters with AGB ejecta in omega Centauri

Takuji Tsujimoto, Toshikazu Shigeyama, Takuma Suda

The origin of a double main-sequence (MS) in omega Centauri is explored. We have shown from theoretical calculations on the stellar evolution that the colors of MS stars are shifte…

astro-ph2006★ 130 cited

The Origin of Carbon-Enhancement and Initial Mass Function of Extremely Metal-Poor Stars in the Galactic Halo

Yutaka Komiya, Takuma Suda, Hiroki Minaguchi +3

It is known that the carbon-enhanced, extremely metal-poor (CEMP) stars constitute a substantial proportion in the extremely metal-poor (EMP) stars of the Galactic Halo, by far lar…

astro-ph2006★ 15 cited

Various Modes of Helium Mixing in Globular Cluster Giants and Their Possible Effects on the Horizontal Branch Morphology

Takuma Suda, Masayuki Y. Fujimoto

It has been known for a long time that some red giants in globular clusters exhibit large star-to-star variations in the abundances of light elements that are not exhibited by fiel…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.